PPT-Status of the ESSnuSB neutrino beam and detector project
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1 Particle Physics with Neutrino Telescopes Uppsala 7 October 2019 T or d E k e löf Upp s a l a Un i v e rs i t y 20191007 PPNT in Uppsala Tord Ekelof Uppsala
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Status of the ESSnuSB neutrino beam and detector project: Transcript
1 Particle Physics with Neutrino Telescopes Uppsala 7 October 2019 T or d E k e löf Upp s a l a Un i v e rs i t y 20191007 PPNT in Uppsala Tord Ekelof Uppsala University . Naba. K . Mondal. Tata Institute of Fundamental Research. Mumbai 400005, India. Brief History. Atmospheric neutrino experiments study neutrinos produced by cosmic ray interactions in the atmosphere.. MINERvA is studying neutrino interactions in unprecedented detail on a variety of different nuclei. Low . Energy (LE) . Beam Goals: . S. tudy . both signal and background reactions relevant . to oscillation experiments (current and future). Jingyu Tang. Institute of High Energy Physics, CAS. NuFact16, . Quy. . Nhon. , Vietnam, Aug. 22-26, 2016. Outline. Brief introduction to the MOMENT. Recent . study progress. Physics potential. R&D efforts at . PPAP Meeting. Birmingham. 15 July 2009. Elisabeth Falk. University of Sussex. Def. current: running or under construction. Outline. Neutrino-oscillation experiments:. what to measure, and how. Accelerator-based experiments. Heavy Neutral Leptons at the SPS. (CERN-SPSC-2013-024 / SPSC-EOI-010. ). On behalf of:. 1. Theoretical motivation. Discovery of the 126 . GeV. Higgs boson . . Triumph of the Standard Model. . The SM may work successfully up to Planck scale !. Neutrino Oscillations in Susan Cartwright Neutrino Oscillations Principles Experimental techniques Neutrino oscillations: Principles The Standard Model contains three neutrinos These can be labelled by flavour as . monitor . for PS. Mariusz Sapinski, . Oliver Keller, . Emiliano. . Piselli. , Bernd . Dehning. - BE/BI. with input from: . Simone . Gilardoni. , Dominique . Bodart. , . Rende. . Steerenberg. ,. W. Farabolini . on behalf of all the CALIFES beam users. 01/121/2015. CLIC Project Meeting #23. 1. Studies repartition with CALIFES and TBM. Test Beam Module : 21 days W. Farabolini. Wake Field Monitors : 48 days R. Lillestol et al.. PPAP Meeting. Birmingham. 15 July 2009. Elisabeth Falk. University of Sussex. Def. current: running or under construction. Outline. Neutrino-oscillation experiments:. what to measure, and how. Accelerator-based experiments. 1. Particle. Physics . with. Neutrino . Telescopes. Uppsala 7 . October. 2019. T. or. d. . E. k. e. löf. Upp. s. a. l. a. . Un. i. v. e. rs. i. t. y. 2019-10-07. PPNT in Uppsala Tord Ekelof, Uppsala University . Applying G4beamline. Tom Roberts. Muons, Inc.. June 27, 2011 TJR. 1. Machine-Detector Interface 2. Outline. Quick Introduction to G4beamline. Why use it for MDI simulations. G4beamline Capabilities Relevant to MDI Simulations. M. Scott Dewey. National Institute of Standards and Technology. Workshop on Next Generation Neutron Lifetime Measurements in the U.S.. How to Measure . τ. n. … . . “Bottle” Experiments:. Direct Observation of Exponential Decay:. in Japan. T. Ishida. Neutrino Section, J-PARC Center, KEK. on behalf of the neutrino beam group . 1. Contents. Neutrino experimental facility at J-PARC. S. tatus of the facility since NBI2012. . Physics reach of T2K / J-PARC to Hyper-K. KEK. for T2K collaboration. Mar.14,2013. n. Telescopes. 2013. Venice. 30min talk including discussion. 1. The T2K Collaboration. (~500 members, 56 institutions, 11 countries). Canada. TRIUMF. U. Alberta.
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